Statistics – Computation
Scientific paper
Nov 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.138..113b&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 138, no. 1, Nov. 1987, p. 113-119.
Statistics
Computation
3
Galactic Structure, Gravitational Collapse, Interstellar Magnetic Fields, Planetary Magnetic Fields, Stellar Evolution, Supermassive Stars, Astronomical Models, Computational Astrophysics
Scientific paper
In this article it is argued that galactic magnetic fields are generated in the earliest moments of galaxy collapse. The model proposes that provided, even if only briefly, a supermassive star is formed early on in the galaxy formation process, this star can produce a strong centrally localized magnetic field which may act as the 'seed' field from which a galactic field can grow. In order to substantiate this model, detailed numerical calculations will be required.
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